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IR Line and Continuum Emission from Bipolar Outflow Sources

Published online by Cambridge University Press:  04 August 2017

Howard A. Smith ,
J. Fischer ,
D. Mozurkewich ,
P. R. Schwartz  and
T. R. Geballe
Howard A. Smith
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
J. Fischer
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
D. Mozurkewich
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
P. R. Schwartz
Affiliation:
Naval Research Lab. Code 4139.5, Washington, DC 20375 USA
T. R. Geballe
Affiliation:
UKIRT, 665 Komohama St., Hilo, HI 96720, USA

Extract

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Most of our understanding of BPF's is based on observations of the neutral and ionized gas in bright, high luminosity sources. Data on low luminosity (L ≲ 30 L⊙) objects has now become more available (e.g. Frerking and Langer, Astrophys. J. 256, 523, 1982) permitting a test of models at this end of the luminosity range. We have performed a series of multi-wavelength observations, emphasizing low luminosity objects.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 343 - 345
Copyright
Copyright © Reidel 1987